000002009 001__ 2009
000002009 005__ 20160701171657.0
000002009 0247_ $$2DOI$$a10.1553/cia150s187
000002009 037__ $$aASTROimport-166
000002009 100__ $$aBriquet, M.
000002009 245__ $$aA comparative study of B-type pulsators and non-pulsating chemically peculiar Bp stars
000002009 260__ $$c2007
000002009 520__ $$aWe carry out a comparative study between a sample of confirmed and well-studied B-type pulsators and a sample of well-studied Bp stars with known periods and magnetic field strengths. Our study indicates that the group of Bp stars is younger than the group of SPB stars and that stars with stronger magnetic fields have much lower pulsation amplitudes. 
000002009 700__ $$a Hubrig, S.
000002009 700__ $$a De Cat, P.
000002009 700__ $$a Aerts, C.
000002009 700__ $$a North, P.
000002009 700__ $$a Schöller, M.
000002009 773__ $$c187$$pCommunications in Asteroseismology$$v150$$y2007
000002009 85642 $$ahttp://esoads.eso.org/abs/2007CoAst.150..187B
000002009 905__ $$apublished in
000002009 980__ $$aREFERD